The table below shows the most common keywords used by the author. The letters in brackets after some keywords denote if the keyword corresponds to Solar Physics (S) or Heliospheric Physics (H).
| Keyword
| Occurrences
|
|---|
| Sun: Corona [S]
| 49
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 25
|
| Sun: Coronal Mass Ejections
| 22
|
| Sun: Magnetic Fields
| 22
|
| Magnetohydrodynamics [S]
| 18
|
| Solar Wind [H]
| 16
|
| Magnetohydrodynamical Simulations
| 9
|
| Waves
| 8
|
| Solar Coronal Holes [S]
| 8
|
| Sun: Flares [S]
| 7
|
| Sun: Filaments [S]
| 6
|
| Physics - Space Physics [H]
| 6
|
| Sun: Heliosphere [H]
| 6
|
| Solar Physics [S]
| 5
|
| Sun: UV Radiation [S]
| 5
|
| Solar Coronal Streamers
| 4
|
| Solar Magnetic Flux Emergence
| 4
|
| Solar Extreme Ultraviolet Emission [S]
| 4
|
| Sun: Photosphere [S]
| 4
|
| Interplanetary Magnetic Fields [H]
| 3
|
| Solar Eclipses
| 3
|
| Solar Optical Telescopes
| 3
|
| Techniques: Image Processing
| 3
|
| Solar Surface
| 3
|
| Solar Activity
| 3
|
| Sun: Magnetic Topology
| 3
|
| Turbulence
| 3
|
| Coronagraphic Imaging
| 3
|
| Astronomy Software
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 2
|
| Solar Coronal Waves [S]
| 2
|
| Methods: Data Analysis
| 2
|
| Sun: Particle Emission
| 2
|
| Sun: Infrared
| 2
|
| Astronomy Data Analysis
| 2
|
| Sun: Evolution
| 2
|
| Magnetic Fields
| 2
|
| Neural Networks
| 2
|
| Interplanetary Turbulence [H]
| 2
|
| Model Selection
| 2
|
| Sun: Physics - Space Physics
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Space Weather
| 2
|
| Sun: Atmosphere [S]
| 2
|
| Quiet Solar Corona
| 1
|
| Plasmas
| 1
|
| Plasma Temperature
| 1
|
| Plasma Density
| 1
|
| Plasma Alfven Waves
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Physics - Computational Physics
| 1
|
| Parallel
| 1
|
| Methods: Observational
| 1
|
| Methods: Numerical
| 1
|
| Methods: Analytical
| 1
|
| Magnetic Reconnection
| 1
|
| 7835)
| 1
|
| Interplanetary Physics: Coronal Mass Ejections (7513)
| 1
|
| Interplanetary Medium [H]
| 1
|
| Instrumentation: Spectrographs
| 1
|
| Flares
| 1
|
| Cross-validation
| 1
|
| Corona [S]
| 1
|
| Computer Science - Programming Languages
| 1
|
| Computer Science - Distributed
| 1
|
| Comets: Individual: Comet C&2011 W3 (lovejoy
| 1
|
| Comets: Individual: C/2011 W3
| 1
|
| Comets: General
| 1
|
| Chemical Abundances
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astrophysics
| 1
|
| Astrophysical Plasma
| 1
|
| Astronomy Planetary-science, Physics, Sociology
| 1
|
| Astronomy Image Processing
| 1
|
| Ultraviolet: General
| 1
|
| The Sun [S]
| 1
|
| Techniques: Imaging Spectroscopy
| 1
|
| Sun: X-rays [S]
| 1
|
| Sun: Waves
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Sun: Shock
| 1
|
| Sun: Rotation [S]
| 1
|
| Sun: Radio Radiation [S]
| 1
|
| Sun: Radio
| 1
|
| Sun: Propagation
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Magnetohydrodynamic
| 1
|
| Sun: Low Coronal Signatures
| 1
|
| Sun: General
| 1
|
| Sun: Fractional Charge States
| 1
|
| Sun: Euv
| 1
|
| Sun: Activity
| 1
|
| Stellar Physics
| 1
|
| Stellar Activity
| 1
|
| Stars: Magnetic Field
| 1
|
| Stars: Coronae
| 1
|
| Stars: Activity
| 1
|
| Space Plasmas [H]
| 1
|
| Solid State: Refractory
| 1
|
| Solar Storm
| 1
|
| Solar Meridional Circulation
| 1
|
| Solar Magnetism
| 1
|
| Solar K-corona
| 1
|
| Solar Filament Eruptions
| 1
|
| Solar F-corona
| 1
|
| Solar Energetic Particles [H]
| 1
|
| Solar E Corona
| 1
|
| Solar Differential Rotation
| 1
|
| Solar Cycle
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Solar Coronal Lines
| 1
|
| Solar Active Region Magnetic Fields [S]
| 1
|
| Solar Active Region Filaments
| 1
|
| Slow Solar Wind [H]
| 1
|
| Shocks
| 1
|
| Shock Waves
| 1
|
| Recombination
| 1
|
| And Cluster Computing
| 1
|
| And Astronomy: Magnetic Reconnection (2723
| 1
|
| And Astronomy: Corona
| 1
|
| Alfven Waves
| 1
|
| Active Solar Corona
| 1
|
| Acceleration Of Particles
| 1
|
| Ionization
| 1
|